INTEGRAL Galactic Bulge Monitoring Revolution 0414: Observation start 2006-03-04 = MJD 53798
Total Observation GTI = 12293 seconds
ISGRI
ISGRI significance mosaic images. Left: ISGRI 18-40 keV. Right: 40-100 keVSources detected > 10σ in each band are marked on the image. The table below lists the fitted position, and statistical positional uncertainty in arcmin returned by the mosaic step of
OSA7
, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 206 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 103 cps ) where available.NOTES: The table is constructed from the
isgri_mosa_res.fits
file - fluxes in the mosaic output are known to be systematically ~10% lower than in the ScW light-curves (see known issues). The systematic noise increases towards the edge of the field of view andNEW
sources < 6σ towards the border of the image may be spurious.
ISGRI Detected Sources 18-40 keV (A) and 40-100 keV (B)Source Name RA dec +/- l b A(cps) +/- sig B(cps) +/- sig ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GX 5-1 270.280 -25.082 0.6 5.073 -1.016 17.0 0.30 57.1 1.3 0.00 5.2 GRS 1758-258 270.304 -25.747 0.9 4.506 -1.365 10.7 0.29 36.7 7.3 0.24 30.5 GX 1+4 263.012 -24.753 0.9 1.932 +4.789 11.8 0.33 36.2 0.0 0.00 0.0 Ginga 1826-24 277.373 -23.795 1.0 9.276 -6.091 18.2 0.55 33.0 6.3 0.43 14.8 GX 349+2 256.434 -36.422 1.2 349.104 +2.750 13.1 0.54 24.3 0.0 0.00 0.0 GX 354-0 262.992 -33.836 1.1 354.302 -0.153 8.3 0.31 26.7 1.1 0.00 4.2 1A 1742-294 266.507 -29.512 1.6 359.555 -0.376 4.7 0.26 18.2 1.9 0.22 8.6 GX 17+2 273.996 -14.037 1.8 16.427 +1.286 35.7 2.33 15.3 0.0 0.00 0.0 H 1820-303 275.932 -30.345 1.9 2.808 -7.916 6.0 0.42 14.2 0.0 0.00 0.0 GX 9+1 270.390 -20.540 2.2 9.070 +1.144 5.3 0.44 12.0 0.0 0.00 0.0 XTE J1817-330 274.413 -33.016 2.3 359.813 -7.980 4.4 0.38 11.5 2.5 0.31 8.0 4U 1722-30 261.891 -30.768 2.7 356.349 +2.315 2.8 0.28 9.9 1.0 0.23 4.5 3A 1822-371 276.438 -37.088 2.4 356.863 -11.279 6.4 0.58 11.0 0.0 0.00 0.0 OAO 1657-415 255.171 -41.688 2.5 344.328 +0.319 14.7 1.39 10.5 0.0 0.00 0.0 4U 1700-377 256.031 -37.870 2.8 347.756 +2.130 5.9 0.62 9.4 2.2 0.49 4.5 GX 3+1 267.015 -26.542 3.3 2.327 +0.781 2.1 0.27 7.9 0.0 0.00 0.0 SLX 1735-269 264.587 -26.981 3.4 0.814 +2.395 2.0 0.26 7.5 1.3 0.22 6.1 1A 1743-288 266.686 -28.879 3.5 0.177 -0.181 1.8 0.26 7.2 1.4 0.22 6.2 SLX 1744-299_300 266.818 -30.011 3.5 359.268 -0.865 1.9 0.26 7.4 0.0 0.00 0.0 GX 13+1 273.619 -17.161 3.5 13.508 +0.115 5.6 0.77 7.3 0.0 0.00 0.0 SLX 1737-282 265.235 -28.320 4.6 359.985 +1.197 1.4 0.25 5.4 0.0 0.00 0.0 IGR J17544-2619 268.632 -26.397 4.8 3.191 -0.389 1.4 0.28 5.2 0.0 0.00 0.0 IGR J17252-3616 261.361 -36.344 4.7 351.475 -0.431 2.2 0.42 5.3 0.0 0.00 0.0 XB 1832-330 278.869 -32.998 5.2 1.502 -11.326 2.6 0.55 4.8 0.0 0.00 0.0JEM-X
JEM-X significance mosaic images. Left: 3-10 keV. Right: 10-25 keV.Note: Sources labelled were detected with in the 3-10 keV image > 10σ and are listed in the table below. Fluxes are extracted at the known catalogue position of the source (i.e. no fitting of the source position is done), with
mosaic_spec
, in two bands: A = 3-10 keV (1 Crab ~ 88 cps); B = 10-25 keV (1 Crab ~ 32 cps).NOTES: Fluxes for light curves are extracted from the images using
mosaic_spec
; The object marked as SLX 1744-299_300 is used to indicate two low-mass x-ray binaries separated by 2.7 arcminutes, SLX 1744-299 and SLX 1744-300; the position for SLX 1744-299 is used, although it can not be ruled out that SLX 1744-300 may dominate the emission some of the time.
JEM-X Detected Sources in 3-10 keV (A) and 10-25 keV (B).Source Name RA dec l b A(cps) +/- B(cps) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== GX 354-0 262.989 -33.835 354.302 -0.150 12.7 1.35 3.7 0.88 GX 3+1 266.983 -26.564 2.294 +0.794 26.5 0.56 4.0 0.31 GX 5-1 270.284 -25.079 5.077 -1.019 97.2 2.11 18.4 1.06
Go back to Bulge home page